On Oct 11, 2011, at 5:31 AM, Roger Burton West <[email protected]> wrote:

> On Tue, Oct 11, 2011 at 05:29:32AM -0500, Captain Joy wrote:
>> I'm not sure I understand; in fact I'm sure I don't.  If you know where on 
>> the ellipse your planet is at at t=0, and you know the semi-major axis and 
>> eccentricity of the orbit, it seems like figuring what angle the planet 
>> moves through each Delta t thereafter should be a fairly simple equation.
> 
> It isn't.
> 
> You can take Hal's approach and slice the orbit into smaller and smaller
> delta-T segments, working out the swept area. Or you can use calculus.
> But neither of these is going to be _simple_.

No, but the angle a planet moves through given its current location on the 
ellipse, semi major axis, delta-T, and eccentricity is an equation that can be 
looked up.
--
Captain Joy
[email protected]

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